Using identical photometric pipelines, the diffuse intracluster light fraction in TNG300 simulated clusters matches WWFI observations for most definitions, although simulated BCG+ICL systems are larger and brighter.
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Photometric analysis of the intracluster light in the TNG300 simulation and wide-field observations
Using identical photometric pipelines, the diffuse intracluster light fraction in TNG300 simulated clusters matches WWFI observations for most definitions, although simulated BCG+ICL systems are larger and brighter.